Fusion in Europe 3 | 2017

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FUSION IN EUROPE NE WS

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Here we are with a second edition of the Fusion Writers Project. This time we took a look into EUROfusion‘s Research Units and discuss rather unusual topics such as proliferation.

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Contents

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2017

Fuel 3 4 8 10 3

2017

Jump on board! Tritium: a challenging fuel for fusion A blanket to fuel fusion Could these shiny metals unlock the power of the sun?

Plasma 12 Fusion neutronics – the biggest gamble in the galaxy? 15 Detecting illusive, yet powerful particles 18 Making the reactor wall smarter 21 The story of sabotage: the Tungsten investigation 24 Domesticate the fire: a crucial step towards fusion energy

Comic

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26 Total eclipse

Whodunit?? Tracing back a saboteur who had killed a beautiful fusion plasma. Picture: B. Simony

44 Imprint FUSION IN EUROPE ISSN 1818-5355

For more information see the website: www.euro-fusion.org

Specifics 28 A snowflake for fusion? 30 The need of the hour: nuclear fusion

Education

How will the energy mix of the future look like? Author Davide Silvagni discusses the next century.

33 Building the future with S.T.E.A.M.

Community 36 The great fusion endeavor

Future

Picture: EUROfusion

39 Preparing early 41 Putting planet earth first? 44 Do we actually need fusion energy at all?

EUROfusion Programme Management Unit – Garching Boltzmannstr. 2 85748 Garching / Munich, Germany phone: +49-89-3299-4128 email: anne.purschwitz@euro-fusion.org editors: Petra Nieckchen, Anne Purschwitz Subscribe at newsletter@euro-fusion.org /fusion2050 @PetraonAir @FusionInCloseUp @APurschwitz

| Fuel | EUROfusion |

© Tony Donné (EUROfusion Programme Manager) 2017. This newsletter or parts of it may not be reproduced without permission. Text, pictures and layout, except where noted, courtesy of the EUROfusion ­members. The EUROfusion members are the Research Units of the European Fusion Programme. ­Responsibility for the information and views expressed in this newsletter lies entirely with the authors. Neither the Research Units or anyone acting on their behalf is responsible for any damage resulting from the use of information contained in this publication.

JUMP ON BOARD! Wow, what a journey! Fusion in Europe continues the ­successful Fusion Writers project in 2017! You now hold in your hands an edition that includes articles from young fusion enthusiasts, born in Australia, Brazil, the U.S., ­India and, of course, many European countries. We know, this magazine is called “Fusion in Europe” but EUROfusion’s research also has links with what is hap­ pening across the pond … and even further beyond. The current edition features 16 essays written by authors who are mostly about to finish their PhDs. Hence, you’ll find more scientific content compared to the 2016 edition. We wanted to take a look inside EUROfusion’s Research Units, wherever we were given the opportunity to do so, and we wanted to hear the news straight from the horse’s mouth. They chose their topics entirely on their own and they were free to speak their mind. We have encouraged our authors to report from their labs in entertaining and understandable ways. And many have succeeded, Žiga and Sarah for instance.

In fact, the boxes made the authors collaborate. For ­i nstance, writers whose essays dealt with, let’s say “tri­ tium”; such as Paul, David and Rodrigo, who, by the way, live on different continents, needed to talk things over. They held intensive discussions to achieve a crisp but ­correct explanation, and finally agreed on a tiny square which is now shared by all of their essays. I would dearly like to thank all of the involved writers and, especially, the cartoonists Amita and Benoît, for their ­incredible commitment and their reliable punctuality. It was a thrilling ride and I am happy that we decided to ­embark on that journey once again. It was a great lesson to learn that even while travelling down the same path twice, you will find something new along the way.

Their secret? Passion. What drives a person to chase neu­ trons, what’s so interesting in checking out the ashtray of a fusion device and, most of all, why should it matter to the world? If the writer is able to share his or her motivation, then we are winning. I have been on that journey for years and I sometimes don’t know where the road is taking me. Unexpected things happen and lead to something new, such as this fresh ­feature: the fusion basics boxes. The author of those packages is Oisín McCormack. He has an extraordinary ability which enables him to explain ­crazy complicated fusion matters in just three minutes. We used that skill and identified fusion topics which come up on a constant basis and which need further explanation. As a result, we ‚forced‘ Oisín to explain them with the help of­ 80 words only, pack them in a box and, hence, take the ­burden off the author’s shoulders. And Oisín did very well.

Anne Purschwitz Editor of Fusion in Europe Picture: EUROfusion

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| Fuel | EUROfusion |

FUSION IN EUROPE

TRITIUM:

A CHALLENGING FUEL FOR FUSION

D

euterium and tritium, two isotopes of hydrogen have, for decades, been considered the fuels for the first generation of fusion reactors. D ­ euterium is practically inexhaustible due to its presence in our oceans. When it comes to the heavier tritium, the story differs considerably. ­Tritium is radioactive, decaying with a half-life of 12.3 years, which explains its ­almost natural lack of existence. In fact, the natural tritium abundance is only around 3.5 kg

Picture 1: Schematic diagram of the tritium breeding inside a fusion reactor. Deuteriumtritium atoms fuse in a hot plasma to produce one atom of helium-4 atom, one neutron and, along with it, energy. The fusion neutrons will escape the plasma and react with lithium atoms present in the so-called breeding blanket to produce atomic tritium. Picture: KIT-ITeP-TLK

Rodrigo Antunes Age: 25 Origin: Portuguese Currently based at:

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Karlsruhe Institute of Technology – Insti­tute­ of Technical Physics – Tritium Laboratory Karlsruhe (KIT-ITeP-TLK) I am currently doing my doctoral ­research at the tritium laboratory in Karls­ ruhe. For many years, I have been interes­ted in the challenges our society will need to face to solve our ever increasing energy­ demands. Nuclear fusion is a promising energy source to which I have been contri­ buting over recent years. Therefore, together with young fusion scientists and engineers,­ I am glad to take part in this special issue of Fusion in Europe.

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THE NEED FOR TRITIUM BREEDING This means we have a problem. How are we able to harness energy created by fusion reac­ tions if one of the fuels (that is to say, 50% of the required reactants) is basically inexistent? The simple answer is: we need to produce our own tritium inside the reactor in the so-called Breeding Blanket (BB). The BB is comprised of lithium-based m ­ aterials and covers the inner wall of the reactor vessel to guarantee tritium production. The reactions between the fusion­­neutrons produced inside the vessel and the l­ ithium atoms present in the BB gene­ rate a­ tomic tritium (Picture 1). Then, another important question arises: how do we process the new-born tritium?

As you can imagine,­ there are a collection of other systems responsible for extracting, processing, ­measuring and injecting the ­fresh­ ­t ritium inside the machine. The designs of these s­ ystems are l­ argely determined by the special properties of tritium.

HOW DO WE HANDLE TRITIUM? Tritium behaves in a similar way to hydrogen: it easily ­permeates metals (especially if hot!) and reacts explosively with oxygen. How­ever, tritium decays, as opposed to hydrogen. In addition, tritium will readily swap w ­ ith hy­ drogen if both meet on the way (the so-­called isotopic exchange). This is of particular con­ cern since tritium p ­ oses a serious threat to

TRITIUM Tritium (also called hydrogen-3) is a radio­ active isotope of hydrogen, and has one proton and two neutrons. It can be produced using lithium to absorb the energetic neutrons created in both fission and fusion reactors. ­Tritium has a rate of decay of about 5% per ­year. It radiates rather weakly externally, how­ ever it is hazardous if ingested, inhaled, or ­absorbed through the skin. It can react in order­ to create dangerous radioactive “tritiated” ­water, which must be controlled to prevent it from contamina­ting local groundwater.

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| Fuel | EUROfusion |

FUSION IN EUROPE Picture 2: Rodrigo Antunes (right) and his colleague working in the “CAPER C” glovebox. This glovebox hosts the experimental setup to separate tritium species from helium with zeolite membranes, which is the core of my PhD. Picture: KIT-ITeP-TLK

human beings if it replaces hydrogen in our biological systems. Therefore, it is very im­ portant to confine tritium within carefully chosen materials and conditions. Polymers, for example, which are present in commer­ cial pumps or used as sealant materials, are not an option. The h ­ ydrogen-tritium replace­ ment would considerably alter the properties of the material. Therefore, a rule of thumb among tritium ­fellows is: no use of polymers, just inor­g anic/metal substances. However, as mentioned above, an additional challenge arises when metallic ducts contain tritium, as it can r­ eadily permeate them. A good trick is to constantly maintain low tritium partial pressures at low temperatures (for instance, around 20°C) in order to control permeation. If this is not possible, it is necessary to imple­ ment tritium permeation barriers. If this is still not sufficient, a glovebox surrounding the tubes containing tritium must be considered.

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WORKING AT A TRITIUM LABORATORY Major tritium laboratories, such as the one at the Karlsruhe Institute of Technology, operate under an air pressure cascade. In this s­ ituation, the pressure inside the lab is slightly lower than the pressure outside in order to prevent tritium being released into the environment. Gloveboxes, which host the tritium processing lines, offer another level of static confinement with an interior pressure slightly lower than that of the lab. The inert atmosphere of these boxes is cons­ tantly refreshed providing an additional ­dynamic confinement. In Picture 2, you can see a picture of my colleague and me working with a glovebox. The box contains the com­ ponents which I require in order to obtain my PhD on tritium separation technologies in view of DEMO. n

All in all, these collaborative ­efforts are necessary­ to ensure that­ ­tritium, along with ­deuterium, will be the fuel of ­commercial fusion power plants.

Tritium will have its own plant In a fusion reactor, most of the sys­ tems­processing the fusion fuels will be ­hosted in the so-called Tritium Plant (TP). Here, the different isotopes can be isolated by d ­ etritiation of gas streams, so that deuterium and tritium can again be fuelled into the reactor. ITER, now under construction in France,­ will have a 35 m tall x 80 m long x 25 m wide TP building. These dimen­ sions are necessar y to house the ­systems responsible for tritium reco­ very, isotope separa­tion, deuterium-­ tritium fuel storage and delivery. However, it should be noted that ITER will only test small mock-ups of tritium breeding elements, with an estimated daily production less than 0.4 g. In con­ trast, the European DEMO, designed to demonstrate tritium self-sufficiency at a reactor scale, may reach a pro­ duction as high as 250 g/day. Thus, in view of DEMO development, ma­ ny European labs are studying and ­designing different tritium breeding, processing and extraction systems. All in all, these collaborative efforts are necessary to ensure that­­tritium, along with deuterium, will be the fuel of com­ mercial fusion power plants.

Rodrigo Antunes

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| Fuel | EUROfusion |

FUSION IN EUROPE

A BLANKET TO FUEL FUSION

ENERGY CAPTURE The energy given off in a fusion reaction c­ omes in the form of highly energetic alpha particles and neutrons. The ­neutrons escape from this confinement and are even­t ually captured by the blanket. The kinetic energy of ­t hese ­particles gets imparted to the structure that captured them, generating large amounts of heat. Heat from the blanket is then transported with a coolant which goes on to drive ­turbines to produce electricity. This part of the reac­ tor works in the same way you might see in a fission or coal power plant. It sounds simple enough, but there are a number of caveats that make this task difficult. For example, even the coolant can cause corrosion of the metal due to the high temperatures involved.

RADIATION DAMAGE When neutrons collide with a solid material,­ they ­scramble the well-ordered atoms in­side of it (imagine the start of a game of pool). Atoms that have been displaced from their original positions can have a profound effect on the properties of materials, causing them to crack or fail ­u nexpectedly. On top of this, when a neutron is ­a bsorbed, a completely ­d ifferent atom can be created in a process known as transmutation. These new atoms further c­ hange a material’s properties and can often be radio­active. As a result, special new materials must be designed that can w ­ ithstand the effects of neutron damage w ithout becoming too radioactive.

Illustration: EUROfusion

Paul Barron Age: 23 Origin: British Currently based at: Manchester, UK

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ture :

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@paulbrrn

In my opinion, if fusion energy is har­ nessed as a viable power source, it will be the greatest scientific achievement in the history of humanity. In addition to the scien­ tific merit, it will also help reduce the world‘s reliance on carbon energy sources. It is for these reasons I have chosen to study a PhD in materials for fusion reactors.

H

arnessing the energy genera-

TRITIUM BREEDING

ted by a fusion reactor while

Not only must the blanket withstand neutron bombardment, it must also be responsible for generating more tritium, required to sustain­­a continuous fusion reaction.

simultaneously generating more ­tritium fuel to sustain the reaction is no easy task. However, that is what is required from a blanket, the

Read more in the article “Tritium: A challenging fuel for fusion” by Rodrigo Antunes on the pages 4 – 7 in this issue.

enormous structure that lines the outside of the first wall.

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There are many different potential designs for the blanket­breeding system and they all h ­ ave advantages and ­d isadvantages. One design ­utilises a molten mixture of lead and lithium to multiply neutrons and breed ­tritium respec­ tively. However, liquid metal flowing around the structure can cause problems as it inter­ acts with the massive magnetic field of the ­tokamak.

PUTTING IT ALL TOGETHER As the blanket is an enormously complex structure, it needs to be tested before opera­ tion. ITER will be built with six ports where­ test blanket modules can be inserted and ­removed. The data gathered from these test components will be vital for continuing to ­d evelop and improve what is arguably the most challenging component of the fusion ­reactor to design. n

TRITIUM AS FUSION FUEL There are many particles that can create fusion energy, but fusing two isotopes of hydrogen – deuterium and tritium – is the easiest to achieve. This reaction produces a high-energy neutron which will escape the plasma and hit the reactor walls. Tritium is very rare, but self-sufficiency can be achieved­ by a “breeding blanket” lining the walls, ­where the escaped neutrons are augmented by a neutron multiplier and react with lithium to produce tritium. This tritium is then extracted and recycled for fuel.

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| Fuel | EUROfusion |

FUSION IN EUROPE

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eutron multiplying materials may help us create all the fuel we need to ensure a fusion powered future.

COULD THESE

SHINY METALS

F THE O R ­ E

­ N? SU

POW

UNLOCK THE

David Tompkins Age: 25 Origin: American Currently based at:

Providence, Rhode Island

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ivate

I am a marketer at Hasbro, Inc. with undergraduate degrees in Marketing and Mechanical Engineering from the Univer­ sity of Pennsylvania. I believe that if you want to make the world a better place, you should build something that is either for kids or for the future. The work being done by ­EUROfusion will make the world a better ­place, and I’m very thankful for the oppor­ tunity to write this piece.

If a strange man were to approach you on the street and offer to sell a jar of mystic metals which would magically allow your car to create all the fuel you could possibly need – you would not be faulted for laughing. However, if a fusion scientist approaches you with a similar offer, you should hear them out. They just might be telling the truth.

Unlike a car, which constantly requires new fuel, a fusion reactor is capable of producing some of the key compo­ nents of its own fuel. In fact, most reactor designs are intended to create at least as much fuel as they consume. This is a rather wise design choice, since tritium, one of the key ingredients in most nuclear fusion fuels, costs about €25k per gram (roughly $30k for my American fellows).

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Rodrigo Atunes and Paul Barron have written excellent articles on the pages 4 – 7 and 8 – 9 in this journal discussing the details of tritium production. Both are very much worth your time.

A JAR OF MAGICAL ELEMENTS COMES IN HANDY

TRITIUM – AN EXPENSIVE, PRODUCIBLE FUEL

While Beryllium and Lead may hold the honors of being tested in upcoming DEMO breeding blankets, Bismuth (picture) is the undoubtedly most colorful of neutron multipliers. Picture: Wikimedia, Hans Braxmeier

We can use the neutron to make one more piece of tritium. At the end of the day, we have the same amount of ­tritium, some extra energy, and a little less lithium, since this is used to make the new tritium. Unfortunately, we have not yet perfected this task. Sometimes, we lose a piece of ­tritium (it’s a slippery one), or our neutrons hit the wrong bit of wall and are wasted. Either way, we slowly deplete our tritium supply.

Making tritium can be tricky in practice, but it is ­straight­forward to explain. The standard fusion reac­tion consumes one bit of tritium and releases one neu­t ron.

Particularly if that jar is full of “neutron multipliers” – substances that, when hit with one neutron, release two neutrons. If we are able to use substances like these, such as the commonly available lead, the rather exotic beryl­ lium or the colourful bismuth, we make it much easier to create all the tritium we need. With neutron multipliers, we trade in a very high-energy neutron for two slightly less energetic neutrons. If we manage to, in turn, com­ bine both of these with lithium – we could actually end up with more tritium than when we started. In fact, ­present designs suggest that we could breed roughly 20 percent­ more tritium than we consume! For reference on the TBR stat which discusses analysis of a breeder blanket module that utilizes beryllium as the neutron multiplier.

THE ROAD AHEAD There are many challenges to overcome when using neu­ tron multipliers (some are quick to melt, some are toxic, etc.), but there is also a tremendous opportunity, namely cheap, clean, and nearly limitless energy. We face a very curious future – where these beautiful and sometimes hazardous metals might help us harness the same reac­ tions that power the stars above. n

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| Plasma | EUROfusion |

FUSION IN EUROPE

Picture: Istock/seyfettinozel

FUSION NEUTRONICS – THE BIGGEST GAMBLE IN THE GALAXY?

Žiga Štancar Age: 27 Origin: Slovenian Currently based at:

Jožef Stefan Institute, Slovenia

Pi ctu

re: pr

ivate

Since I was a child I was captivated by the world of science, motivated by things we cannot yet explain. Working in neu­tronics, I am still mesmerised by the fact that one can successfully recreate the phenomena observed in large fusion devices by simu­ lating an immense number of individual sub-atomic particles. I consider it a great­ honour to contribute my part to the mosaic of fusion energy research by way of my endeavour s in neutron and plasma physics.

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Illustration: Žiga Štancar

W

ho would have thought that simulating games of chance could be ­considered a serious scientific pursuit, giving birth to a technique ­capable of solving complex problems in physics? The story of the Monte Carlo method begins in the underground labs of the Manhattan Project and continues with modern supercomputers running neutron transport calculations. For more than 60 years, the use of this method for advanced neutronics codes has been aiding mankind in our quest to harness fusion energy. 13


| Plasma | EUROfusion |

FUSION IN EUROPE

Neutrons are an inevitable part of fusion. They are born within fusion reactions in plasmas composed either solely of deuterium ions, or of a mixture of deuterium and t­ ritium. Being chargeless, neutrons escape from the ­plasma chamber, hitting the walls and penetrating deep into the tokamak’s structure. Neutrons are able to change the nuclei of the atoms they interact with – the consequences are either ­v ital to the envisioned fusion device’s electricity ­production or destructive. It is therefore crucial to be able to predict how m ­ any neutrons are born in the plasma and in what manner they interact with their surroundings. To uncover the collective ­impact of neutrons, scientists perform complex neutron transport computations using sophisticated com­ puter codes. These codes rely on the Monte ­Carlo method, and enable us to simulate the individual behaviour of billions of neutrons by drawing upon large quantities of random numbers. What the last century deemed science fiction has become science fact thanks to the rapid increase in the ­world’s com­ putational power.

FROM THROWING BAGUETTES TO A CASINO IN MONACO The question of whether random events are able to lead to concrete conclusions was first answered in the eighteenth century by an influential French scientist, Count Buffon. He proved it was possible to deter­mine the value of pi by tossing baguettes onto a lined tile floor. Thus, the probability that a baguette will land on a crack is proportional to the mathe­ matical constant. Moreover, he showed that the pi estimate was more accurate with every additional baked ­delicacy thrown over his shoulder. It was not until the Manhattan Project, designed for the devel­ opment of nuclear weapons, that the fundamentals of the Monte Carlo method were estab­l ished by ­some of the brightest minds of that era. The method is named after a casino in Monaco, since it enables complex physics problems to be solved by repeated random sampling, a process akin to playing games of chance.

ANYONE INTERESTED IN A GAME OF DICE? The Monte Carlo method was applied to neutron physics from the very start, more specifically to the

study of neutron travel through radiation shielding material.­Although the theory of neu­tron transport has been well estab­lished using the Boltzmann equa­ tion,­it proves d ­ ifficult to solve analytically ­without significant simplifications. This is ­especially­true for complex systems such as a ­tokamak. In contrast, modern Monte Carlo simu­lations treat determi­nistic problems by first finding a probabi­listic analogue. This means the lives of neutrons in a fusion device, known as histories, are individu­ally ­simulated from birth to absorption or loss from the system. The ­specifics of a neutron’s p ­ ath – place of birth, direc­ tion of movement, distance travelled and type of inter­actions – are determined by ­random samp­ling of well-known physics phenomena. One can imagine the sampling process to be akin to t­ hrowing­dice, the outcome of which defines the r­ esult of an event the neutron encounters. For e­ xample, if a neutron is bound to interact with an atom in the walls of the ­tokamak, we can use the know­ledge of the probabi­ lity of absorption, scattering or an inelas­tic s­ cattering reaction and determine which one of the three will occur in the simu­lation – all based on the result of the roll of a dice.

DETECTING ILLUSIVE, YET POWERFUL PARTICLES

I

n commercial fusion power plants, the energy deposited by neutrons into a blanket surrounding a plasma will provide

power to the national grid. JET has shown that deuterium and tritium create a promising fuel for fusion, producing neutrons travelling at around 40,000 km/s. It is essential that we are able to predict neutron intensities reliably in order to opti­mise a future fusion power plant

A MULTITUDE OF NEUTRON HISTORIES The number of neutrons generated in a toka­ mak p ­ lasma is enormous. To get to an accurate represen­tation of reality, several billions of neutron histories need to be simulated using Monte Carlo neutronics codes. In order to combine this with complex ­tokamak geometry, we need to perform a huge n ­ umber of “dice rolls”, a task that is made pos­sible by the ­i ncrease in computational resour­ ces. The con­c lusions drawn from a multitude of single ­neutron simulations are analysed to obtain knowledge of quantities of i­ nterest. For e­ xample, the amount of tritium breeding, wall heating, ­material embrittlement or dose rates. It is somewhat counterintuitive to imagine that throwing dice might give us insight into not only what is going on in a fusion reactor, but also how galaxies have evolved or whether it is going to rain tomorrow. ­However, Monte Carlo simulations re­peatedly prove to be a powerful tool in providing answers to ­problems that are dif­ficult to solve analytically. n

WHAT MAKES NEUTRONS INTERESTING? In a fusion device neutrons are both instrumental and problematic. High-energy neutrons released during ­f usion reactions may escape from the plasma and ­deposit energy in the blanket. Converting this energy into ­heat will be the most promising way to power the national grid. The measured number of neutrons produced in ­f usion reactions provides information about the power output, as well as the rate of fuel consumption. In addi­ tion, neutrons are used to breed the tritium necessary to fuel a self-sufficient ­reactor.

See also the article „A blanket to fuel fusion“ by Paul Barron on pages 8 – 9 n in this edition.

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Chantal Nobs Age: 26 Origin: British Currently based at: Abingdon,

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Oxfordshire @Chantal_Nobs In March 2017, towards the end of my PhD at the University of Brighton, I started working at the Culham Centre for Fusion Energy. I wanted to help solve the challenge of fusion energy because it has the poten­ tial to provide huge benefits to society. To ensure continued progress in fusion I think it is important to share my research with the wider community.

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| Plasma |

FUSION IN EUROPE

HOW CAN WE MEASURE WHAT WE CANNOT SEE? The diameter of the neutron is on the femtometre scale (10 -15 metres). For comparison, the diameter of a strand of human hair is on the micrometre scale (10 -6 metres), thus a billion times larger than the ­d iameter of a neu­ tron. It is difficult even to comprehend something this small, but the nature of neutrons makes them even more ­challenging to measure. Conventional radiation detectors rely on the c­ ollection of charge­to provide information about the radia­t ion detected. Unlike protons and elec­ trons, n ­ eutrons ­have no charge; and unlike alpha, beta and gamma ­radiation, neutrons do not induce a charge in mate­rials. To measure neutrons we must instead use an indirect p ­ rocess and look at the way in which they ­interact with other materials, a field known as neutronics (introduced in the Fusion in Europe March 2016 edition). Neu­t ron activated materials emit gamma rays with charac­­teris­t ic energy­“fingerprints” thus providing the identification of the atom excited ­during activation. By detecting these gamma rays, along with simulations pre­ dicting how the atom may ­have been e­ xcited by neutron interactions, it is possible to ­deduce the neutron spectrum.

WHO WRITES THE INFO BOXES?

Picture: private

VERDI – THE COLLABORATIVE DETECTOR

Deuterium-Tritium Reaction

Neutron Interaction with Iron

Picture 1: An illustration of nuclear reactions inside a tokamak device. Bottom left: inside the plasma, d ­ euterium and tritium fuse together in a high temperature plasma releasing a neutron and an alpha particle. Bottom right: Neutrons cause activation by way of interactions with atoms, such as iron. This results in transmutation to other elements, such as manganese and the release of characteristic gamma rays using radioactive decay processes.

NEUTRONS Neutrons are subatomic particles with slightly more mass than a proton, but with zero electric charge. The chemical and nuclear properties of an atom depend on the number of protons (P) and neutrons (N) it has. In a fusion plasma, deuterium (1P, 1N) fuses with tritium (1P, 2N) to produce helium (2P, 2N), one neutron (1N), and 17.6 MeV of energy. The energy is divided between the helium (3.5 MeV) and the neutron (14.1 MeV), but since the neutron has no charge is able to escape the magnetic field that confines the plasma.

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HOW NEUTRONS WILL HELP TO PREDICT FUSION PERFORMANCE When neutrons collide with materials they may ­i mpart some of their energy, trans­ forming and exciting the atoms within the material. This process is known as activa­ tion, and is illustrated in Picture 1. Activated ­m aterials then undergo radioactive decay. ­Activation is also a tool that may be used to in­d irectly m ­ easure the neutron produc­ tion rate in ­f usion. The energy spectrum of neutrons is used to gather important plasma parameters such as the temperature. In the blanket of a fusion p ­ ower plant, the spectrum informa­tion may be used to predict the rate of tritium ­production.

The high temperatures, intense magnetic fields and high neutron fluences of a fusion environment p ­ resent signi­ ficant challenges when it comes to neutron detection. The UK, Greece and Italy have c­ ollaboratively developed the VERDI detector ­(Picture 2). It will transport mate­ rial samples inside the fusion device blanket, where they will be bombarded by neutrons. The samples will then be ­removed and placed in front of a conventional radiation detector. Carbon has a high melting point (over 3000°C), so by ­encapsulating material samples in a carbon shield the VERDI detector can be ­placed much closer to the plasma core than existing neutron detectors. Detecting neutrons is just one of the many challenges that must be overcome in nuclear fusion. It takes multiple experts from several nations to c­ ome together to solve even comparably small tasks in the huge quest for fusion energy. n

Oisín McCormack Age:

30

Nationality: Irish Currently based at:

Padova, Italy

I am a PhD student at Consorzio RFX and I work with developing new techniques for plasma temperature diagnostics. Fusion is the only field I have ever considered dedicating my life to. I enjoy spreading the good word of fusion, seeing the expression of wonder on other’s faces as they realize the grand impor­tance of it. To me, communication is an essential part of being a good scientist.

Picture 2: A prototype of the VERDI detector, prior to initial testing.

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| Plasma | EUROfusion |

FUSION IN EUROPE

MAKING THE REACTOR WALL SMARTER

SMART ALLOYS – A POSSIBLE SOLUTION Smart alloys might provide an answer to this demanding question. Alloys are materials consisting of two or more compounds, for ­e xample, metallic compounds. Often they are designed to improve the materials‘ pro­ perties. Steel for example is an alloy made up mostly of iron, but containing a few percent of chro­m ium (Cr) and other elements that alto­ gether improve the corrosion resistance of the ­material.

T

here are a lot of “smart” devices that support you in your daily life. But “smart” surely also serves fusion. Smart alloys are a pos­sible­ way of preventing the release of ­radioactive material in the event of an accident when operating future fusion reactors.

W-based self-passivating ‘smart alloys’ are intended to suppress the WO3 formation and thus passivate the oxidation properties compa­ red to pure W. The alloy’s smartness consists of its ability to adapt to two kinds of operation scenarios. When the smart alloy comes into contact with oxygen, its elements form a dense protective oxide layer at the surface and thus prevent tungsten mobilisation.

Janina Schmitz at the linear p ­ lasma device at Forschungs­ zentrum Juelich. The experiment tests material for future fusion reactors. Picture: Tobias Wegener (CC-BY-NC-SA 3.0)

Janina Schmitz Age: 25 Origin: German Currently based at:

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re: pr

W – THE MATERIAL’S SOLUTION? ivate

Forschungszentrum Juelich (FZJ)/Ghent University The idea of creating a Sun - like ­power generation source on Earth can only be ­r ea­lised by the joint efforts of fusion ­researchers from all over the world. With my PhD work within the Fusion Doctoral College framework, I want to contribute to this aspiring project. At FZJ, and elsewhere in Europe, we are developing tungsten-ba­ sed smart alloys for future ­f usion power plants like DEMO. My research is focus­ sed on the plasma compatibility of smart alloys.

18

In its normal operational mode as plasma-­ facing material, preferential sputtering of light alloy elements causes the depletion of these alloying elements at the surface. It forces the alloy to behave like pure W during reactor ­operation.

Tungsten (W) is currently the prime can­ didate for the plasma-facing wall of a fusion experiment. It features a high melting point and low tritium retention. Another factor that meets the requirements of a future ­f usion­ ­reactor wall, are its low sputter yields. Sput­ ter­yield is the term for the number of sput­ tered or ­dispersed target atoms per incoming projec­t ile. A unity sputter yield means that each i­ ncoming atom sputters one target atom. ­Despite these advantages, there are also some­ drawbacks in using W as plasma-facing ­material: W is in­herently brittle and its duc­tile­ -to-brittle-transition temperature even ­increases along with high temperature as well as neutron irradia­tion. In order to improve the material’s ductility and enhance its toughness, different approaches must be investigated.

THINGS SHOULD NOT GO LOCA In order to build a safe fusion experiment, we must consider extraordinary events in additi­ on to the operational scenario. These might put additional constraints on the development of plasma-facing components (PFCs). In case of a so-called LOCA (loss-of-coolant-accident), the cooling of the first wall fails and, as a con­ sequence, the wall temperature may rise up to 1200 ºC for several months. With additional air ingress, W oxidises easily and radioactive volatile tungsten oxide (WO3) is formed. This requires elaborate measures to prevent this gas from being released into the environment. In order to finally achieve an intrinsically safe ­f usion operation, it would be best to entirely avoid the mobilisation of the wall material.

NEUTRON ACTIVATION Neutron activation is where energetic neu­trons induce radioactivity in a material. Free neu­ trons are captured by atomic nuclei, pushing them into an excited state. These atoms then release decay radiation in order to return to a stable state. The neutrons produced in fusion reactors are not confined to the plasma and can hit the wall material, which will predo­ minantly be made of tungsten in future devices. Continuous activation will degrade the tungsten, which will then need to be replaced and disposed of as low-level radioactive waste.

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| Plasma | EUROfusion |

FUSION IN EUROPE

THE STORY OF SABOTAGE: THE

TUNGSTEN INVESTIGATION

ADVANCED W MATERIALS FOR DEMO Smart alloys are possibly a solution in the event of LOCA. However, for DEMO, the next step after ITER and the first fusion power­ plant, the need for long-lasting PFCs with ­additional stable mechanical properties ­during plasma operation is just as important. The

20

Origin: French Currently based at:

Aix-en-Provence, France

­ evelopment of advanced materials designed to d meet the demanding requirements of a ­f usion opera­t ion is progressing. Material solutions ­tailored to ensure low erosion and long lifetime PFCs are moving forwards. Yet their behaviour in ­regimes beyond regular reactor operation must be examined more closely. At FZJ, we are currently also working on ­improving the various drawbacks of pure W. We are also looking into the use of tungsten fibre­ reinforced composites (Wf/W) as a solu­tion to the inherent brittleness. At the same time, we are developing self-passivating smart alloys in order to improve the material during LOCA events. Ultimately, our efforts must be combined and a composite designed which has suitable pro­ perties for both the operational and accidental reactor scenario, and which is geared to any eventuality. n

ict u

re: p

rivate

In four months I will finish my PhD in nuclear fusion (hurrah!). I believe that fusion is capable of solving the energy crisis and I want everyone to know about it. A teacher once told me “If you can’t explain your job in a way that anyone can understand, then you don’t understand it yourself”. Writing about fusion in an accessible and illustrated way is challenging but so fun and fulfilling!

THE FACTS CARTOONIST

Benoît Simony Age: 26 Origin: French Currently based at: Aix

France

c Pi

For the currently most promising alloys, Cr is used as passivating element, while yttrium (Y) serves as an active element to improve self-passivation. Oxidation tests carried out at Forschungszentrum Jülich (FZJ) demons­ trated a significant improvement in oxidation suppression for the WCrY system. And initial plasma tests at the linear plasma device PSI-2 showed no impact on the oxidation behaviour.

Age: 26

HOW SPECIAL FORCES COMBINE TO CATCH PLASMA KILLERS

The smart alloy is exposed to fusion conditions, Picture: Andrey Litnovsky

At the same time, the self-passivation p ­ roper­ties of the smart alloy should remain ­un­affected by the plasma impact as the a­ lloying elements in the bulk material remain.

Sarah Breton

P

AUTHOR

Ultimately, our efforts must be c­ ombined and a composite designed which has suitable properties for both the opera­tional and a ­ ccidental reactor scenario, and which is geared to any eventuality.

en Provence,

tu re: B

. Simony

I just finished my PhD in passive neutron coincidence counting on radioactive waste drums. Although it is not applied to fusion, I am also very interested in it, and more ­generally, in wider topics of physics. Further­ more, I like to use my passion for drawing in order to illustrate physical phenomena and the life of researchers.

It had all started well. We managed to ­heat­up the reactant in order to make the expected fusion reaction happen: in this case, deuterium, an hydrogen isotope. We initiated a current into the tokamak, that strange doughnut-shaped reactor. Very strong magnetic fields are used to en­sure that hot particles don’t touch the inner wall of the tokamak. Finally, we were very ­pleased when we witnessed that the deu­ terium started to warm up, became ionized and converted into a gas called plasma. Ion and electron temperatures were increased ­successfully in the centre of the plasma, up to 150 million Kelvin. Fusion is happening right now. So far so good.

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| Plasma | EUROfusion |

FUSION IN EUROPE

The W investigation, allegory, Cartoons: B. Simony

THE SUSPECT AND THE TIMELINE

The control room

THE DEAD OF THE PLASMA

THE EVIDENCE

There are about twenty people glued closely to the screens in the control room. One of us, the pilot, makes the ­decisions. He or she watches the live footage from ­inside the tokamak. All of the plasma parameters had been finely tuned before the experiment started. Now the ­plasma c­ ontrol system manages everything automati­cally. The pilot is simply in charge of the emergency ­button to immediately stop the operation in the event the ­machine may be damaged.

Fusion experts like us measure several plasma parameters: current, temperature, density, radiation. In this instance, the radiation emitted by the plasma had i­ ncreased over time. This is the signature of one suspect: Tungsten, or W. We know where this tungsten comes from, a special area called the divertor. It is designed to receive a lot of energy.

Meanwhile, another part of our team is responsible for monitoring the experimental signals from previous ­experiments. But suddenly, the core temperature starts to drop. This is exactly what we don’t want: a decline in the plasma temperature! This surely would kill the highly desired fusion reaction. Immediately, the system responds and increases the cen­ tral heating function. But the temperature keeps dropping. Within a couple of seconds, the plasma dies, releasing enough energy to damage the walls. The camera shows a sudden light, like a flash, then it all goes dark. In the control room, nobody speaks. Wordless question marks hang in the air. Something went wrong. What happened?

22

More on divertors: see also the article „A snowflake for fusion?“ by Carrie Beadle on the pages 28 – 29.

More on Tungsten: see also the article „Making ths reactor wall smarter“ by Janina Schmitz on the pages 18 – 20

Tungsten is a popular fusion material because of its high temperature resistance and its low erosion rate. Un­ fortunately, some erosion is still caused by the energy that ends at the divertor. W enters the plasma, but is so heavy it does not get fully ionised. This means that not all the electrons are torn away from the nucleus, and that causes W to radiate. And W is the only species in the tokamak that has this property: it has to be the material used.

So now, we have found the saboteur. And we have to stop it. To prevent this situation from occuring again, we ­simply must understand how tungsten managed to ­radiate so much that it made the plasma collapse. We decide to ­reconstruct the timeline of W impurities, just like in a police investigation. First, we gather together the infor­ mation we have about the temperature, density and rota­ tion profiles, radiation levels, and especially the radiation ­distribution in the plasma. Aha, here is our first important clue: the radiation first appeared at the edge of the plasma. But after a couple of seconds, all of the emitted radiation is derived from the centre of the plasma. This means that W travelled from the edge to the centre. And this is what has caused the core temperature to drop and the plasma to collapse. But how did W travel through the plasma? W was transported, W had accomplices.

PERSONS OF INTEREST AND MODUS OPERANDI The measurements are necessary to reconstruct W’s time evolution, but not sufficient to figure out the transporta­ tion of W. We need to use another tool: simulation. The W transport obeys known mechanisms and equations. Infor­ matic codes have implemented these. The inputs are W‘s accomplices, the Persons of Interest: temperature, den­ sity­and rotation profiles. The outputs are the coefficients that quantify how far and how fast W is transported. But W also impacts the evolution of temperature and density,­ and radiation as we have seen before. There are many feedback loops to be simulated if we wish to reconstruct the modus operandi. The combination of several codes

is called integrated modelling. It is a very complex and sensitive tool. Simulating just a few seconds of plasma can take days, or weeks, depending on the level of complexity.

HOW A THREE SECONDS SABOTAGE REQUIRES MONTHS OF WORK As a result, we have to gather our Special Forces, a team made up of experts with various scientific backgrounds in order to finally catch the saboteur and to figure out its modus operandi. This is what fusion and the reali­sa­tion of fusion energy is about. We, as scientists, are ­dealing with phenomena that have not yet been inves­­ti­g ated. We are pioneers … and, more often, even detectives. n

TUNGSTEN Materials inside a fusion reactor must be ­able to operate for a long time under neutron bombardment and hot plasma attack. Tungsten is the most promising material for use as ­plasma facing components. Tungsten is a robust, rare, metal chosen for its very high melting point (3422 °C), low tritium reten­tion, and low erosion rate. However, even rela­ tively small amounts of eroded tungsten dust are able to poison the plasma, cool it down and cause a disruption, which may result in ­serious ­damage­­ to the machine.

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| Plasma | EUROfusion |

FUSION IN EUROPE

DOMESTICATE THE FIRE: THE POWER EXHAUST PROBLEM The particles and heat flux coming from the plasma core are channelled downstream along magnetic field lines to a region called the “divertor”. Divertor targets must withstand power fluxes in the order of several MW/m 2 in steady state conditions, and up to 1 GW/ m2 during intrinsic instabilities of the plasma. This is comparable to the friction that occurs during re-entry of a spacecraft into the Earth’s ­atmosphere. This holds true just for the stea­ dy-state regime, while plasma instabilities can lead to a hundred times the expected power loads of the plasma during ~0.5 millisecond.

A CRUCIAL STEP TOWARDS FUSION ENERGY

F

usion energy is created by merging t wo atoms in a

very hot gas, called plasma, with temp er atures around 150 mil­lion Kelvin. This ex­ treme ­s cenario takes place in a reactor with a doughnut-­

Tungsten target exposed to hydrogen plasma in the linear machine Magnum-PSI. Picture: DIFFER

like geo­m etry, called a tokamak. Plasma-­surface interactions pose one of the biggest

Renato Perillo

­o bstacles for ­f usion experi-

Age: 27

Eindhoven (NL)

Institute,

re :

u

Currently based at: Differ

ments. The future reac­tor wall

t Pic

Origin: Italian

p r iv ate

I am a driven PhD student wor­ king within the Plasma Edge Physics and ­Diagnostics group at the Dutch Institute for Fundamental Energy Research. I combine numerical simulations with experiments, addressing the issue of power exhaust in a fusion reactor. I do believe fusion energy is the most promising energy source for the future. Working day by day in such a stimula­ ting environment is the best thing that could have happened to me.

24

INTERDISCIPLINARY RESEARCH AS A KEY TO SUCCESS Since the early ‘80s, scientists have been trying to reduce the heat flux on the target by in­creasing the gas pressure in the divertor ­region. The plasma is cooled down throughout its path to several thousands of Kelvin due to radiation, momentum transfer and volume ­recombination processes. In this way, the ­heat loads become sustainable for the material. This phenomenon is called “plasma detach­ ment”. In order to fundamentally understand detachment and PSI in a tokamak, various dis­ ciplines, such as material sciences, control and mechanical engineering, plasma physics and chemistry have to work together properly.

FROM MAGNUM-PSI TO ITER

rios in which the wall loads are

The linear plasma machine Magnum-PSI, ­located at DIFFER (Eindhoven, NL), is capable of mimicking the plasma-surface interactions foreseen for ITER. The excellent diagnostics accessibility provides accurate insights into­ the mechanisms occurring in both the ­exposed material and in the plasma located in the ­vicinity of the target.

more benign. One way to cool

WANTED IMPURITIES IN THE DIVERTOR

mate­r ials have to with­s tand incredible heat and par ticle fluxes. Scientists are currently investigating plasma scena-

the plasma down is by means of impurity seeding.

the influence of nitrogen seeding on a hydrogen plasma, focusing on the plasma chemical­ ­p rocesses occurring in such scenario. So far, experiments and numerical simulations­ deliver promising results while achieving a more comprehensive understanding of p ­ lasma detachment in a fusion reactor. In the end, this w i l l be a key factor in ma k ing this technology feasible within the second half of this century. n

Experiments in tokamaks over the course of the last two decades have shown that the injec­ tion of gas (so-called impurities) ­into the diver­ tor region leads to an enhanced ­detachment. At DIFFER we are currently pursuing such ­experiments. In particular, we are investigating

Renato Perillo (right) in the control room. Picture: private

PLASMA INSTABILITIES A fusion plasma is an extremely hot elec­ trified gas which naturally wants to expand. It is suspended in a strong magnetic field designed to keep it from touching the chamber walls. As the temperature and pressure builds, the plasma forms areas of increasing turbulence, called instabilities, that must be controlled. There are many different types and sources of instabilities that may cause plasma disruption. The worst instabilities are able to eject streams of hot plasma out of the magnetic confinement, severely eroding the wall materials.

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| Comic | EUROfusion |

FUSION IN EUROPE

5

TOTAL ECLIPSE

4

Idea: Luiz Trevisan Cartoon: Amita Joshi 26

1

6

2 3

Luiz Trevisan

Amita Joshi

Age: 34

Age: 28

Nationality: Brazilian/Italian Currently based at: Houston

Pi ctu

Origin: Indian re: pr

ivate

I‘m a chemical engineer in the com­

Currently based in: Germany

Pi ctu

re: p

rivate

As they say, ‘A picture speaks a

mercial fossil fuels sector and fascinated

­thousand words’. Keeping this quote in mind

by fusion, science, industry and history. Not

I worked as illustrator for this edition of

only technologies but engineering careers

­EuroFUSION too and tried to convey technical

will need to evolve in order to develop in­

stuff through a comic strip to make it lucid. This

dustrial fusion. I hope that humanity will

was my second year with EuroFUSION team,

succeed in this great journey of creating

I wish the bond strengthens. I thank ­Anne

universal and balanced access to energy.

again to give me this opportunity. Cheers!

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| Specifics | EUROfusion |

FUSION IN EUROPE

A SNOWFLAKE FOR FUSION?

PROBLEMS AT THE EDGE Two of the biggest scientific and technological challenges facing ITER and DEMO are associated with plasma-wall interaction. Firstly, how to minimise the heat load on the target plates. Secondly, how to prevent impurity particles from entering the core plasma and causing heat loss. For this reason, such troublesome particles should be kept to a finite, well-defined area.

BEYOND THE LIMITED CONFIGURATION Early tokamaks achieved this aim using a limiter – typi­ cally a rail extending a short way inwards from the inner wall of the tokamak. In this configuration, it is relatively easy for the impurity particles to re-enter the core plasma. A solution was proposed as early as in the 1950s, split the flux surfaces at a certain point. The field lines will cross each other and end at two divertor plates, some distance away from the last closed flux surface, keeping the core plasma “safe and clean”. However, it wasn’t until the 1980s that this more complex configuration started to be used in fusion devices.

DETACHING THE PROBLEM

The Swiss Tokamak à configuration variable (TCV) from above. Picture: Christophe Roux/EUROfusion

Carrie Beadle Age: 23

Center, Lausanne

Plasma

e:

ur

Currently based at: Swiss

t Pic

Origin: British

p ri vate

I am a PhD student studying plasma turbulence in the outermost region of the tokamak via numerical simulation. I find fu­ sion plasma physics exciting because it has so many different aspects, challenges and problems to be solved! My article is about the problem of overheating materials where they interact with the plasma and how we can change the magnetic field configuration to keep vessel walls from melting.

A

snowflake might not be the first thing you associate with a hot fusion plas-

ma. But it is a concept designed to handle the heat where the plasma touches the vessel wall. It is not surprising that this task presents technical difficulties. How­ ever, the scale of the problem is remar­ kable: the predicted heat load on the ITER targets is greater than that on the soil beneath a launching rocket!

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The diverted configuration also tackles the tremendous heat load problem. No material would be able to withstand such harsh conditions. The greater distance between the target and the flux surface allows density and temperature gradients to form along the magnetic field lines, thus redu­ cing the temperature at the target to well below that in the core. The heat load can also be reduced by either ­spreading the same total heating power over a greater plate area, or by radiating more heat before it reaches the target. This requires a strongly radiating “cushion” of dense neutral gas between the target and X point. It remains very diffi­ cult to simultaneously reach the detached regime for the targets and maintain the high-confinement mode, which optimises the core plasma performance.

ADVANCED DIVERTORS ITER must operate in both high confinement mode and the detached regime. The challenge is to maintain the ­detachment front in a stable way. It is here that the shape of the flux surfaces close to the target becomes important. So, we need a new concept: advanced divertors. These are magnetic configurations in which there is not one but two magnetic X points. The second X point ­modifies the angle at which the field lines arrive at the target as well as the change in separation between the flux sur­faces as they approach the target. Current experiments are trying to find the magnetic field which provides the most effective heat load reduction.

Limited vs diverted configuration. The limited configuration is shown on the left, with the limiter itself in blue, last closed flux surface in bold red and flux surfaces in red. On the right is the diverted configuration, with the target in blue and magnetic surfaces as before. Snowflake flux surfaces on TCV.

IT’S JUST THE BEGINNING One such advanced configuration is called the “snow­ flake”. It is named after its 6-fold symmetry, achieved by a ­s econdary X point close to the primary X point. Researchers have discovered that this reduces the heat drastically. The area that receives the heat becomes much larger. Also, the d ­ istance along a field line from the X-point to the target is now longer, allowing a much greater drop in temperature along the line. It is clear that we need to understand the ­effect of divertor geo­ metry on the heat load. Theoretical modelling of diver­ ted geometries is just beginning, but already there are hints that first principles models can ­r ecover ­r esults of experiments such as those carried out on Tokamak à con­figuration variable (TCV). So, watch this space! n

DIVERTOR A divertor is the in-built vacuum cleaner of a fusion reactor and is situated along the chamber floor. Build-ups of helium ash and impurities in the plasma must be removed during operation. These heavier particles are pushed to the edge of the plasma by centrifugal forces, where they escape through a specially designed magnetic “gap” at the bottom of the plasma and fall into the divertor. The divertor shape and materials are also constructed to bear the brunt of the heat load from the plasma, thus protecting the surrounding walls.

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| Specifics | EUROfusion |

FUSION IN EUROPE

THE NEED OF THE HOUR: NUCLEAR FUSION

s a child, I witnessed innumerable incidents of load shedding in Delhi, especially during summers. This meant no electri­city at home and studying by candlelight for

hours. Even today 24/7 power supply remains a dream that is unfulfilled. Just ­imagine, there are around 396 million ­people­with no access to electricity in India! Around 75% of the world population is living in developing countries with energy demands that are expected to surpass that of developed nations in the next 50 y­ ears. My big q ­ uestion

Picture: Istock/Sean Kuma

A

SI S I CR A REALITY

NOT MYTH

is: “How do we tackle this energy crisis?” We will be running out of non-renewable ­resources in the next 40 to 80 years. But, coal, oil and natural gas currently supply most of the world’s energy. CONFINEMENT IS KEY

THE DILEMMA OF CHOICE

Priyanjana Sinha Age: 25

Greifswald, Germany

e:

ur

Currently based at:

t Pic

Origin: Indian

p ri vate

I am a PhD student, but also a ­science enthusiast with a passion for ­w riting.­ I believe that nuclear fusion un­d eniably holds the key to solving the current global­ energ y­ crisis. EUROfusion presents a ­perfect platform for young researchers like me to s­ peak out and dispel the misconcep­ tions as well as raising awareness about nuclear fusion amongst the general public.

30

The general scepticism about nuclear energy is well known. Like most countries, India has also witnessed raging controversy regarding the suitability of nuclear power as the solution to ever growing energy requirements. I too was drawn into this debate and thus developed a strong desire to contribute something towards the promotion of clean and abundant energy. It engendered in me a deep interest in nuclear physics and engineering. It was only during my master’s studies that I understood in-depth the prospect of employing fusion power as an ­a lmost inexhaustible source of energy for­ ­future generations. Now, I am proud to work at one of the most developed fusion experiments in this world: the stellarator Wendelstein 7-X (W 7-X).

Fusion reactions take place at high tempera­ tures of around 10 keV (~100 million Kelvin) where the fuel is in a fully ionised state, also called plasma. The particles have a large ther­ mal velocity with a tendency to escape from the machine. Hence, some method of confine­ ment of particles is essential. Magnetic field confine­m ent using high powered magnets is one of the solutions. Tokamaks and stel­ larators, two t­ ypes of fusion experiments, are both based on this concept.

See also the article “A snowflake for fusion?” by Carrie Beadle on the pages 28 – 29.

A recent publication in Nature Communi­ cation, by Prof Thomas Sunn “from my ins­ titute”, the Max Planck Institute for P ­ lasma Physics, highlights the success ­achieved in W7-X. Sunn Pedersen discussed how he and his colleagues managed to tackle the chal­ lenges.

THE COMEBACK OF STELLARATORS – WENDELSTEIN 7-X

A LIKELY SAVIOUR: CONNECTION LENGTH

In the past, research into stellarators has been overshadowed by interest in the other con­ cept, the tokamak. However, recent ­ad­vances in computational power and engineering ex­ pertise have revived it. So, the inauguration of Wendelstein 7-X (W7-X), the world’s newest stellarator, has put stellarator research back on the fusion table.

The main obstacle in reaching high power­ densit y in fusion devices is the limited capability of the divertors. Divertors are the ashtrays of fusion experiments and need to withstand immense heat and particle loads. My present goal is to develop of special ­magnetic configurations that should help to manage the heat flux. They will be tested in

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| Education | EUROfusion |

FUSION IN EUROPE

BUILDING THE FUTURE WITH

S.T.E.A.M. C CE NG R A I H I T T E NO NE H NLE C OG R I EYN

Picture: private

Inside the stellarator Wendelstein 7-X. Picture: Christophe Roux/EUROfusion

an operational campaign in W7-X. This should further assist us in comprehending the impact on the exhaust physics in a stellarator. Once the riddle of tackling the tremendous power exhaust from fusion plasma has been solved, we will have moved one large step closer to a fusion power plant.

THE SILVER LINING: NUCLEAR FUSION The previous operation phase of W7-X has concluded in March 2016 and delivered ­promising results. We found parameters, for example, for plasma temperatures and den­ sities, that e­ nhance the performance of a ­stellarator ­plasma, exceeding predicted values from simulations. There is, of course, still a lot of research that must be done before nuclear fusion b ­ ecomes a viable commercial option. Nevertheless, I feel like I am participating in the creation of the future solution for the demanding energy needs of the world. Fusion will, I hope, one day create energy for every­ body. n

32

Fusion will, I hope, one day create energy for everybody.

G

T

TOKAMAKS vs STELLARATORS Tokamaks are the most well developed reactor type due to their simple flat magnetic coil design. They have an induced electric current that confines particles on a helical path, but this current also means pulsed operation and results in unwanted instabilities. Stellarators have a complicated twisted coil design, which has been made possible thanks to modern computer modelling. These twisted coils produce a natural helical path thus avoiding the current instabilities and resulting in a much desired steady-state operation.

here is a great demand for techni­ cally skilled people in our information-­

driven society. S.T.E.A.M., an acronym that stands for Science, Technology, ­Engineering, Art and Maths, is an inter-

The Ev3storm roboter is one of the models the school children learned to programme. Picture: The Lego Group

disciplinary approach to learning. Being both physicists and robotics instructors, we decided to launch a project for young enthusiasts, specifically including girls, who are traditionally underrepresented in the sciences. 33


| Community | EUROfusion |

FUSION IN EUROPE

NEXT GENERATION OF INNOVATORS In the end, we achieved our aims, we have prepared the next generation of innovators. By teaching science and technology literacy, we have increased the level of interest in all those who might, one day, wish to work in fusion or other future-relevant subjects.

CREATE-EVALUATE-IMPROVE “Transformers visit my school” is a scheme ­designed for primary and middle school pu­ pils. With the help of Lego Mindstorms ro­ botics kits, the children have learned how to design and construct a robot, attach sensors, think in terms of algorithms and program the tiny machine.

Can there ever be a connection between Art and S.T.E.M.? According to Leonardo Da Vinci, we need to “realise that everything connects to everything else”. Those addi­ tional skills make sciences applicable and ­innovative in real life. Mathematical concepts such as ­s patial awareness or geometry are ­easily ­approached by art while cultivating a basic scientific tool: the power of observation. ­C hildren become open minded and quickly assimilate new ideas.

According to Leonardo Da Vinci, we need to ΄realise that everything connects to everything else΄

G

Irene Papa Age: 28 Origin: Greek

Pi ctu

Currently based at: Athens, Greece

CONNECTING ART AND S.T.E.M.

Nowadays, success results from what we are able to do with knowledge acquired. Hence, in addition to preparing our future workforce, it is essential to spread the benefits of S.T.E.A.M. education.

34

I learnt to take risks. I evaluated my constructions and improved them.

Another fascinating aspect was that ignorance aids ­learning and further improvement. By this we mean, f­ ailures are considered to be part of the discovery process thus ­leading to a better approach. “I learnt to take risks. I evaluated my constructions and improved them”, states Lucas Lenard, a sixth grade primary student.

ELEMENTARY KNOWLEDGE

Engaging children from an early age in spe­ cial processes, enables them to culti­v ate and c­ apitalise on their own interests and, moreover, their ­curiosity. By watching them confront the technical difficulties with the Lego robots, we understood how they­learned to investigate.

As was mentioned earlier, it is not news that girls are underrepresented in scientific and technological fields. This will have an impact on the future staff pool. Young women are often engaged in traditionally “girly” stuff. Early interven­t ion with S.T.E.A.M. subjects encourages them to parti­cipate. Our project boosted the self-confidence of f­ emale partici­ pants as they took on the technical chal­lenges. We rea­lised that when girls overcome their fear of failure or non-qualification, they even gear up. In m ­ any cases, they were chosen to be team leaders during our c­ ompetition. In summary, it is important that these positive projects do not remain single events only. Key influen­ cers, such as parents, teachers and specifically ­women-leaders should further encourage girls to continue in technical fields.

Lucas Lenard

The partakers even approached difficult scien­ tific concepts, such as the physics of sensors, more easily. Hands-on ­a ctivities are used to fill the gaps left by traditional education methods. Our participants enjoyed their practical challenges including building, testing, programming and troubleshoo­ ting. They worked excitedly and creatively­ and let their team spirit guide them. Our role, in the mean­t ime, was to mentor and lead them, allowing the young ­engineers to take their own initiatives and creative­risks, and to explore their different levels of expertise and imagination. We discovered that the satis­faction of accomplishment was a further motivation to the teams. They finally realised that science is everywhere and ready to be discovered!

S.T.E.A.M. C CE NG R A I H I T T E NO NE H NLE C OG R E Y NI

GIRL‘S PIPELINE ISSUES

“I enjoyed that we worked as a team in the Robotics First Lego League in Greece. Everyone had a distinct role, but we needed to colla­ borate and share our ideas in order to complete the tasks”, says nine year old Eudoxia Karlati-­ Koufopoulou.

Key influencers, such as parents, teachers and specifically women-leaders should further encourage girls to continue in technical fields.

re: p rivate

I am an undergraduate physicist and a Robotics instructor. Wanting to pursue a career in fusion, I believe that the answer to the question of safe and clean energy is written in the stars! Fusion and its attractive prospects promises a better future, so I would like to participate in the diffusion of this effort.

THE FOUNDATION OF A VISION Technical education can be applied widely and creatively in order to overcome stereo­ types. Working practically with children and encouraging them to explore, enables them to gain a deeper understanding of technolo­ gical fields. Science has simply become more relevant to them. Indeed, our pupils gained additional skills. They finally realised that S.T.E.A.M is a key way to make their own and others’ lives better". n

Nikos Moraitis Age: 30 Origin: Greek Currently based at: Athens, Greece

Pi ctu

re: p rivate

I am a physicist and my field of exper­tise is Medical Physics. I have been fasci­nated by the subatomic world and the power of the nucleus. Fusion is a great example of this power and I think we all must corporate in order to achieve the promising future of vast and clean energy.

35


| Community | EUROfusion |

FUSION IN EUROPE

A QUEST FOR CLEAN ENERGY Our use of fossil fuels has an accelerating countdown ­t imer. Either we completely ­deplete our available re­serves or we damage­ the ­environment just enough to prevent ­human society from continuing as we know it. We have to find alternative sources of clean ener­ gy, whatever they may be. As the head of the Electron Cyclotron Section of ITER and ­advocate of fusion energy, Dr. Mark Hender­ son, puts it: ”We are addicted to carbon. We have to prove, as a s­ pecies, that we are collec­ tively intelligent enough to ­prevent our own extinc­t ion.” Fusion looks like a promising answer.

THE GREAT FUSION

ENDEAVOR

We are addicted to carbon. We have to prove, as a species, that we are collectively intelligent enough to prevent our own extinction. Dr. Mark Henderson

I

t has been said that the nuclear ­fusion conundrum will be solved ­within 30 years … but they have been saying that for the last 50 years al­ready. Now, we humbly expect the first feasible fusion power plant prototype to start operations sometime in the 2060s. Producing electricity from fusion­is the greatest engineering and scientific challenge of our century. A scientific journey that is greater than achievements such as the building of the Great Pyramids or the Great Wall of China, or landing on the Moon … and this time, humankind depends on it.

36

Mark Henderson

37


| Future | EUROfusion |

FUSION IN EUROPE NOT THERE YET Fusion power plants will create artificial stars and become the clean energy source that will power our way of life in the future. But we are not quite there yet. At the moment, it takes a lot of energy to confine the plasma and a lot more to heat it up to the temperature r­ equired for fusion to occur. At this time, we are ­building ITER to prove that we will be able­ to obtain a net gain of energy output from­ a ­f usion reaction, sometime in the next 20 ye­ ars. Then, DEMO, a prototype power plant, will be built in order to transform the excess output fusion energy into usable electricity, based on everything we learn from ITER.

that “as fusion scientists we have the chance­ to impact the future of the hundreds or thousands of generations to come.”

PREPARING EARLY

As fusion scientists we have the chance to impact the future of the hundreds or thousands of generations to come. Dr. Mark Henderson

LONG TERM COMMITMENT

FUSION IS PART OF OUR FUTURE

Generations of scientists have dedicated their whole careers to fusion research, but there is still a long way to go. The end goal is so far into the future that those who finally make fusion happen may not have even been born yet. The tens of thousands of scientists and individuals working towards fusion today are well aware that they might not be remembered in ­t hirty or forty years, and that is okay. Believing in fusion is looking beyond the importance and the lifetime of our generation. Mark presumes

Nuclear fusion is the epic scientific quest of our time. “We have to face the fact that fusion is extremely complicated”, warns Mark. “We need to orient the scientific community and the population towards it. Otherwise, look at the consequences”. Fusion is one of our best hopes, as a species, to have a sustainable and reliable n ­ ear-limitless source of clean energy within the 21st century. “I believe we will have multiple clean sources of energy in the future: solar, wind – but fusion will be the basis”, says the ITER expert. n

Picture: Istock/PashaIgnatov

Diogo Elói Aguiam Age: 27 Origin: Portuguese

Lisbon, Portugal @diogoaguiam

ct ure

Thom Dixon

Pi

Currently based at:

Age: 28

: pri vate

T

he prospect of a fusion power plant is edging closer to reality. Work is underway to ensure that these plants will be designed to mitigate low-level proliferation risks.

https://daguiam.github.io https://www.linkedin.com/in/ diogoaguiam/

I am an electronics engineer currently doing a PhD in the Advanced Plasma ­Science­ and Engineering programme. ­I develop micro­ wave reflectometry diagnostics that aid other physicists understanding plasma behavior in nuclear fusion research. I advocate for Open Science and thank ­EUROfusion for the support in publishing Open Access.

38

The tokamak pit of ITER some years ago. Pictures: Eyesteelfilm

Origin: Australian Currently based at: Macquarie

University, Sydney @thomdixon

Pi ctu

re: pr

ivate

I am interested in communicating how emerging technologies reshape the world and challenge the status quo. Fusion power will do away with the limits of energy supply and fundamentally rewrite our understanding of power generation. Though this is not without risk, the risks are minimal and need to be communicated before they are misunderstood.

39


| Future | EUROfusion |

FUSION IN EUROPE RISK SCENARIOS The breakout scenario has long been a concern for the international community but it’s never been a major ­concern when it comes to fusion research. There simply haven’t been significant levels of fertile material in fusion. However, w ­ ith fusion power plants looming on the horizon, the risk calculus will change. Research and development is now underway to mitigate these low-level risks.

Dr Richard Kamendje, Responsible Office of the EUROfusion ITER Physics Department Picture: EUROfusion

Dr Richard Kamendje from EUROfusion, who previously dealt with proliferation issues at the IAEA, anticipates that over the coming decades the inter­ national community will need to incorpora­ te s­ ome s­ afeguards to ­m itigate the low-level risks in fusion.

WHAT ARE THE LONG-TERM PROLIFERATION SCENARIOS FOR FUSION? As the largest fusion experiment on Earth, ITER will test breeding blankets for the p ­ roduction of tritium. One ­f uture breakout scenario involves a state that introduces ­fertile material to the breeding blankets. However, not only would doing this have implications for the tritium breeding ratios – every cubic centimetre counts – but it would alter the ­power consumption of the plant and the detec­t able signatures of the tritium. Both of these­ changes­ can be tracked by satellites using ­c urrent ­technology and the presence of fertile material would quickly be discovered.

PUTTING PLANET EARTH FIRST? REVISITING THE DEBATE ABOUT THE FUTURE OF GERMANY’S ENERGY SUPPLY

Another breakout scenario is the introduction of fertile material into the coolant flow. Again, this scenario can be mitigated by ­monitoring changes in background radiation. While further research and development is re­quired to confidently mitigate this risk, there is plenty of time left to do so and ITER will pro­vide the perfect opportunity.

There is an awareness of the risks, they’re manageable and the international community is taking steps to anticipate them. Dr Richard Kamendje

TRITIUM IN NUCLEAR WEAPONS Fusion boosted bombs fuse deuterium and tritium as a trigger to spark lots of early neutrons, which chain-react to make the primary fission explosion more efficient and about twice as powerful. This is a relatively simple weapons technology, and it is suspected that North Korea currently have this type of bomb. A pure fusion bomb is a hypothetical weapon. In comparison with fission fueled bombs, weapons using 100% deuterium-tritium fuel could more easily evade current non-proli­ feration measures.

40

SAFEGUARDS BY DESIGN New designs for nuclear power plants are sent to the IAEA for approval and must incorporate safeguards in the de­ signs. While there are no current designs for fusion power plants, there is little doubt they will go through a simil­ ar process. The next 20 – 30 years will see the research, development and design of such reactors. At each step along the way, the long-term low-level risks will be known and planned for. ITER has enabled international scientific collaboration on a scale that has rarely been seen before. This stands in mar­ ked contrast to competitive nuclear weapons research and the construction of their supporting facilities. Careful and considered research over the c­ oming decades will ensure that fusion remains the low-level proliferation concern it always has been. n

Picture: Istock/Iukbar

T

he future scenario in Germany appears obvious: Rene­wable energies are to be expanded and conventional power s ­ tations

are to be closed down. Simply add on a few storage systems and power grids and the German energy transition is complete – but is it really that simple? 41


| Future | EUROfusion |

FUSION IN EUROPE WHERE TO ENERGISE? For decades, the German population has feared n ­ othing more than a nuclear disaster. After the Fukushima ­accident Chancellor Merkel and her government finally decided to close down all of the remaining nuclear power plants within eleven years.

Even in the best case scenario it is more likely that Ger­ many will need to multiply the level of power generated from renewable sources by ten or twenty times the cur­ rent rate. Wagner also warns about the underestimation of dimensions of storage systems and their operational limitations.

2010

THE STAGNATING DEBATE

But climatologists have been warning us about climate change since the early 70s. As a result, the government has also been forced to develop a plan designed to help decrease CO2-emissions until 2050. As a consequence of this, and in order to reduce greenhouse gases, Germany has also decided to shut down its fossil fuel power plants.

Lignite Hardcoal

IMPOSSIBLE GOALS? Now the country has to fight a battle on two fronts. ­Renewable energies primarily replace another CO2-free one, viz. nuclear, while the use of fossil fuels decreased slightly (see Graphic). This is one of the reasons why it is very probable that the next climate change goal in 2020 will not be met. Additionally, in order to compensate for the remaining nuclear power plants, Germany must ­theoretically double its wind power capabilities. To achieve­ these aims, the rate of expansion of renewable energy had to be about one order of magnitude larger (see www.energy-­ charts.de).

2016

Gas Renewables Nuclear

DON’T BE TOO OPTIMISTIC!

42

Germany’s energy mix before Fukushima and now. The red component represents the climate impact of each source. (Based on www.energy-charts.de and VDI 2007)

TO PREVENT THE WORST CASE SCENARIO On the other hand, we might also stick to the current ­strategy, which means: we continue to hope that sometime within this century renewable energy will be sufficient for our needs. However, if we are to fail, the result would be a simple one: the power supply, even that of 2100 will be a dirty and noxious one, if sufficient at all. That would be putting “Planet Earth last”. n

NEW IDEAS FOR THE FUTURE OF ENERGY Given the problems explained above, I think, we need to embark upon a renewed debate of Germany’s energy ­future. In an unbiased discussion, we need to figure out an energy mix that will minimise the risks for both humans and the environment.

The famous banner of the anti-nuclear movement at a protest-camp against coal mining near Cologne, Germany in 2017. Is it in times of climate change still legitimate to reject nuclear fission and fusion?

In the long run, nuclear fusion should, together with ­renewable power, play a crucial role. It may be able to ­supply the growing energy demand world-wide much more adequately than a complex system based ONLY on renewable sources. Anyway, we must accept that ­f usion will not help us to reduce the CO2 emissions before 2070 or even later. Though emissions have to be rapidly d ­ e­creased already in the coming years, if we want to succeed in ­stopping climate change. Fusion can help in the longer run to meliorate the two major disadvantages of wind energy and Photovoltaics, which is low power density and intermittency.

In an unbiased discussion, we need to figure out an energy mix that will minimise the risks for both humans and the environment.

Fabian Wieschollek Age: 23 Origin: German Currently based at: Garching

near Munich, Germany fb.me/Fabian.Wieschollek

ct ure

Pi

Is it possible for Germany to be fully powered by rene­ wable energies by the end of this century? There are a few optimistic, yet non-reviewed studies, like Greenpeace’s “Plan B” or “Kombikraftwerk2” produced by the Agency of ­Renewable Energies. They predict that it can be ­achieved by way of relatively small efforts, by installing plants, storage and backup s­ ystems. A nyhow, most of t hese st ud ies have­­critical issues: they ignore, for­­ example, changing weather cond itions or assume a n ­u nrealistic decrease in the amount of energy consu­ med. I propose to con sider the calculations made by Fritz Wagner, retired German plasma physicist and ­former director at the IPP. He has generated simu­ lations for a fully renewable supply that also takes into considera­tion sector-coupling or an inter­national power grid.

About 71 % of Germany’s population (according to an ­Emnid study from 2017) agrees that climate change is one of the biggest threats to today’s society. But in 2016, 70 % of Germans also wanted to avoid nuclear fission according to a study from YouGov. Fusion seems fascinating but does not play a major role: for example, when Wendelstein 7-X created its first hydrogen plasma in 2016, fusion was a trending topic in the German news for about a week. However, in the government’s decla­ ration on the energy policy, fusion is not even mentioned. So, nuclear power of any kind appears to remain s­ omething of a hot potato in this country. In most cases, it is only associated with potential risks and nuclear leftovers. The contradiction between phasing out nuclear power and ­attaining climate goals is often downplayed by politicians, independently of their party membership (see both the government‘s declarations and the party programmes of CDU, SPD, Alliance 90/The Greens, The Left). Meanwhile, the European Union is keeping its nose out of this struggle. The Parliament in Brussels has declared that each country is free to choose the method of supply it prefers, just as long as the EU member states accomplish the international climate goals.

I personally have come to the conclusion that we ini­ tially should focus on phasing out the use of fossil fuels for ­power. Nuclear power will be necessary as long as the ­problems of pollution are as present as they are today. I know that continuing to use nuclear as a source of power will be a tough decision. The full argumentation would explode beyond the scope of this article.

: priv at e

I am a student of Physics and I will be ­initiating my master’s thesis in fusion re­search by the end of this year. I intend ­entering into the theoretical fields, because the mathematical description of nature has always been an interesting challenge. For me, convincing society of visions of a sus­ tainable future is more exciting than maths itself. That’s why I have enjoyed debating this topic even since my days at school.

43


| Future | EUROfusion |

FUSION IN EUROPE

DO WE ACTUALLY NEED FUSION ENERGY AT ALL? A NEW ENERGY CONSUMING LIFE-STYLE

W

ill it be possible to use

My grandparents generation will probably be remembered as the one that experienced the most incredible changes during their lives: they were born in a society where phone boxes­ were the only way to make calls, where travel­ ling was a luxury reserved for the rich, where clothes were washed only by hand. Now, their generation uses mobile phones, travels by p ­ lane and owns washing machines. The ­c hanges that my grandparents have experienced­ during their lifetime are not without con­ sequences for our society. The world energy consump­t ion has grown enormously in the past 90 years, increasing to seven times that of 1930. This dramatic jump is not only related to the ­population growth. The world‘s per capita energy-consumption has doubled the value from 1930: hence, our life-style has become much more energy-consuming in a very short period of time.

just renewable energies

to reduce the world‘s fossil fuel consumption? Could fusion power help to reduce the world‘s CO2

emissions? S ometimes t he ­simplest questions are the most important – and the most difficult – to answer. A small excursion into recent energy problems and cutting-edge energy predictions may help to put these questions into the right focus and to provide proper answers.

HIGH FOSSIL FUEL CONSUMPTION: NEED FOR AN ENERGY TRANSITION

PARIS CLIMATE AGREEMENT The 2016 Paris Agreement is a major international accord on tackling climate change, supported by almost 200 countries. It aims to restrict the global average temperature to less than 2° C above pre-industrial levels, mainly by way of cutting greenhouse gas emissions. 2° C is seen to be a tipping point, beyond which irreversible climate changes will occur, leading to a devastating rise in sea levels, extreme droughts and wildfires. Fusion could provide an essential source of zero emission energy needed to achieve the goals of the ­Paris Agreement.

44

Picture: EUROfusion/Shutterstock

To satisfy this thirst for energy, fossil fuel consumption was increased dramatically. Coal, oil and natural gas rapidly began to domi­ nate the energy market. Now everyone is fami­ liar with the effects of this “energy revolution”: the increased emission of greenhouse gases is ­a ffecting the natural environmental balance that has ruled on Earth for more than 100,000 years. A relentless global warming process is causing the ice to melt and the climate to change and has resulted in disastrous impacts on our lives. At the same time, the concentration of fossil fuels in few regions (Middle East, R ­ ussia etc.) is seriously undermining geopolitical stability. Hence, a society with low fossil fuel consumption has become a fundamental goal that must be achieved in order to restore the world‘s natural and geopolitical stability. The Paris agreement of 2016 is pushing towards this aim, even if it has some limitations.

45


FUSION IN EUROPE RENEWABLE ENERGIES ALONE ARE NOT ENOUGH In this context, renewable energies play a cru­c ial role. Wind farms, solar panels, bio­ mass, geothermal and hydro power plants ­represent valid energy sources that can help to reduce fossil fuel consumption. Nevertheless, a ­socio-economic study of EUROfusion pub­ lished in 2016 estimates that by 2100 renewable energies will cover 68 % of the total electricity­ production, while 21 % will still be provided by fossil fuels and 11 % by nuclear fission. This scenario sets low CO2 emission targets, a c­ on­d ition that is helping the penetration in the market of renewable energies and does not consider fusion energy to be an option at all. Hence, it seems clear that renewable energies alone will not be able to completely conquer this energy transition.

A FULL ENERGY TRANSITION COULD BE ACHIEVED IN 2100 The same EUROfusion socio economic study­ also analyses a different scenario, one which con­ siders a drastic reduction of the world per capita energy consumption, a low CO2 emission target and the first fusion power plant connected to the grid to be in operation by 2070. Considering that we are talking about developments that may ­be implemented in 50 years‘ time, we should ­always

Davide Silvagni Age: 24 Origin: Italian

Germany

ct ure

Pi

Currently based at: Garching,

: priv at e

I am a former student of the Euro­pean Master of Science in Nuclear Fusion and Engineering Physics and I recently started a PhD at the Max Planck Institute for Plasma Physics in Garching. As an energy engineer, I believe that engineers should develop “appropriate technologies” for mankind. Fusion is one of these, since it may help to reduce CO2 emissions and the high fossil fuel dependency of our society, as I explain in my article.

46

2100 – FUSION failure Nuclear fission 11%

EUROPEAN CONSORTIUM FOR THE DEVELOPMENT OF FUSION EN EUROPEAN CONSORTIUM FOR THE DEVELOPMENT OF FUSION ENERGY

Fossil fuels 21%

Renewable energies 68%

2100 – with FUSION

REALISING ELECTRICITY REALISING FUSIONFUSION ELECTRICITY Institute of Plasma Physics Academy of Sciences of the University of Cyprus Czech Republic

Austrian Academy of Sciences

Ecole Royale Militaire Austrian Academy of Sciences Laboratory for Plasma Physics

Ecole Royale Militaire LaboratoryAcademy for Plasma Physics Bulgarian of Sciences

Bulgarian Academy of Sciences Croatian Research Unit

Croatian Research Unit University of Cyprus

Technical University of Denmark

Technical University of Denmark University of Tartu

Technical Research Centre University of Tartu of Finland

Commissariat à l’énergie Technical Centre atomiqueResearch et aux énergies of Finland alternatives

Commissariat à l’énergie atomique et aux énergies alternatives

FRANCE GERMANY

GERMANY

Max-Planck-Institut für Plasmaphysik

Max-Planck-Institut für National Center for Scientific Plasmaphysik Research "Demokritos"

National Center forCentre Scientific Wigner Research for ResearchPhysics "Demokritos"

Wigner Research Centre for Dublin Physics City University

Agenzia nazionale per le nuove tecnologie, l’energia e lo Dublin City University sviluppo economico sostenibile

Agenzia nazionale per le nuove tecnologie, l’energia e lo sviluppo economico sostenibile

Lithuanian Energy Institute

Institute of Plasma Physics Lithuanian Institute and LaserEnergy Microfusion

Institute of Plasma Physics and Laser Microfusion Instituto Superior Técnico

Institutofor Superior Institute AtomicTécnico Physics

Institute for Atomic Physics Comenius University

Jožef StefanUniversity Institute Comenius

Centro de Investigaciones Energéticas Medioambientales y Tecnológicas

Centro de Investigaciones Energéticas Medioambientales y Tecnológicas Swedish Research Coubcil

Swedish Research Coubcil

SWITZERL AND THE NETHERLANDS

UNITED KINGDOM THE NETHERLANDS UKRAINE

UNITED KINGDOM

AU STRIA

AU STRIA BELGIUM

BELGIUM BU LG AR IA

BU LG AR IA CROATIA

CROATIA CYP RUS

CYP RUS LIC CZECH REPUB

Institute of Academy of Czec

CZECH

Fossil fuels Nuclear fission 5% 6%

Nuclear fusion 14%

DENMARK

DENMARK ESTONIA

ESTONIA FINLA ND

FINLA ND FRANCE

GER

Renewable energies 75%

Source: D. Silvagni

be cautious with such timelines. None­the­­­less, this study has interesting results: it p ­ redicts that, in 2100, 75 % of the total electricity production will be generated by renewable ener­ gies, 14 % by fusion power plants, 6 % by nuclear fission and only 5 % using fossil fuels. These estimations are telling us something ­quite intuitive: if we will bring about a drastic reduction of our per capita energy consump­tion, if we aid the development of renewable ener­ gies and if fusion power plants are able to start operating soon enough, the energy transition could be achieved fully by 2100. Fusion energy, then, would not be a childish tantrum of stub­ born scientists that do not want to throw in the ­towel, but it seems it will be necessary in order for our society to restore the world‘s natural and ­geopolitical stability. n

GERMANY

LITHUANIA

SPAIN

GERMANY GREECE

LITHUANIA POLAND

SPAIN SWEDEN

GREECE HUNG ARY

POLAND PORTUG AL

SWEDEN SWITZERL AND

HUNG ARY IRELAND

PORTUG AL ROMANIA

Our partners:

IRELAND ITALY

ROMANIA SLOVAKIA

ITALY LAT VIA

SLOVE NIA SLOVAKIA

LA

Jožef St

SLO

Our partners:

FRANCE

FR ANCE SPAIN

S


This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014 – 2018 under grant agreement No 633053.

Many more facilities are involved in the European fusion research. The map shows only those for which EUROfusion contributes to the operation costs.

ISSN 1818-5355


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